Pattern formation mechanisms in motility mutants of Myxococcus
Transcription
Pattern formation mechanisms in motility mutants of Myxococcus
Pattern formation mechanisms in motility mutants of Myxococcus xanthus Jörn Starruß∗ ,1, 2 Fernando Peruani † ‡ ,1, 3 Vladimir Jakovljevic,4 Lotte Søgaard-Andersen,4 Andreas Deutsch,2 and Markus Bär5 1 These authors have contributed equally to this work. Center for Information Services and High Performance Computing (ZIH), Technische Universität Dresden, Zellescher Weg 12, D-01069 Dresden, Germany 3 Laboratoire J.A. Dieudonné, Université de Nice Sophia Antipolis, UMR 7351 CNRS , Parc Valrose, F-06108 Nice Cedex 02, France 4 Max Planck Institute for Terrestrial Microbiology, Karl-von-Frisch Straße 10, D-35043 Marburg, Germany 5 Physikalisch-Technische Bundesanstalt, Abbestraße 2-12, 10587 Berlin, Germany (Dated: September 12, 2012) 2 Formation of spatial patterns of cells is a recurring theme in biology and often depends on regulated cell motility. Motility of the rod-shaped cells of the bacterium Myxococcus xanthus depends on two motility machineries, type IV pili (giving rise S-motility) and the gliding motility apparatus (giving rise to A-motility). Cell motility is regulated by occasional reversals. Moving M. xanthus cells can organize into spreading colonies or spore-filled fruiting bodies depending on their nutritional status. To ultimately understand these two pattern formation processes and the contributions by the two motility machineries, as well as the cell reversal machinery, we analyze spatial self-organization in three M. xanthus strains: i) a mutant that moves unidirectionally without reversing by the Amotility system only, ii) a unidirectional mutant that is also equipped with the S-motility system, and iii) the wild-type that, in addition to the two motility systems, occasionally reverses its direction of movement. The mutant moving by means of the A-engine illustrates that collective motion in the form of large moving clusters can arise in gliding bacteria due to steric interactions of the rod-shaped cells, without the need of invoking any biochemical signal regulation. The two-engine strain mutant reveals that the same phenomenon emerges when both motility systems are present, and as long as cells exhibit unidirectional motion only. From the study of these two strains, we conclude that unidirectional cell motion induces the formation of large moving clusters at low and intermediate densities, while it results into vortex formation at very high densities. These findings are consistent with what is known from self-propelled rod models which strongly suggests that the combined effect of self-propulsion and volume exclusion interactions is the pattern formation mechanism leading to the observed phenomena. On the other hand, we learn that when cells occasionally reverse their moving direction, as observed in the wild-type, cells form small but strongly elongated clusters and self-organize into a mesh-like structure at high enough densities. These results have been obtained from a careful analysis of the cluster statistics of ensembles of cells, and analyzed on the light of a coagulation Smoluchowski equation with fragmentation. PACS numbers: Formation of patterns of spatially organized cells is a recurring theme in biology. These processes often depend on regulation of cell motility. For instance, in metazoans it provides the basis for organ formation during embryogenesis and, in single-celled eukaryotes such as Dictyostelium discoideum, it is essential for the formation of fruiting bodies. In bacteria, regulated cell motility is essential for the colonization of diverse habitats as well as for the formation of multicellular structures such as biofilms and fruiting bodies. These pattern formation processes can be self-organized. For example, Dictyostelium discoideum [1, 2] regulates cell aggregation and multicellular organization by secreting and sensing the diffusive signal cAMP. In Myxococcus xanthus, on the ∗ These authors have contributed equally to this work. authors have contributed equally to this work. ‡ Corresponding author: [email protected] † These other hand, rippling patterns and the highly complex cellular reorganization leading to fruiting body formation are controlled by a non-diffusing signal, the C-signal [3]. Interestingly, collective effects and self-organization can also occur, to a certain extent, in the absence of an explicit signaling mechanism. For instance, hydrodynamic interactions can induce large-scale coherent motion of swimming cells, as recently observed in Bacillus subtilis[4, 5], and a density-dependent diffusivity can lead to aggregation patterns as recently suggested to occur in Escherichia coli and Salmonella typhimurium [6]. M. xanthus is a gliding bacterium that has been used as a model system to study pattern formation [14], bacterial social behaviour [15], and motility [16]. The rod-shaped cells of the bacterium M. xanthus move on surfaces in the direction of their long axis using two motility machineries, type IV pili, which requires cell-to-cell contact for its activity beacuse it is stimulated by exopolysaccharides on neighboruing cells [17] (giving rise S-motility), and the gliding motility apparatus that allows cells to move 2 FIG. 1: Pattern formation at various packing fractions η, 6 hs after spotting a drop of bacterial suspension on an agar surface. First row corresponds to the non-reversing A+ S− Frz− mutant that moves only by means of the A-motility system (these three panels have been taken from [7]). Second row corresponds to the non-reversing A+ S+ Frz− mutant that moves with both the A- and S-motility system. At high cell densities, the mutants A+ S− Frz− and A+ S+ Frz− form large moving clusters that turn into vortices at sufficiently high packing fractions. Third row corresponds to the wild-type A+ S+ Frz+ strain that moves with both the A- and S-motility systems and cells are able to reverse their moving direction. The A+ S+ Frz+ mutant self-organizes into a mesh-like structure at high density. in isolation [18] (giving rise to A-motility). Force generation by the A-motility system has been suggested to rely on either slime secretion from the lagging pole [22], or on focal adhesion complexes distributed along the cell [23]. Cells occasionally reverse their gliding direction with an average frequency of about once per 10 min and the reversal frequency is controlled by the Frz chemosensory system [19]. In the presence of nutrients, M. xanthus cells form coordinately spreading colonies. Upon depletion of nutrients M. xanthus cells initiate a complex developmental program that culminates in the formation of spore-filled fruiting bodies. Both motility systems as well as reversals are required for the two cellular patterns to form, i.e., spreading colonies and fruiting bodies. It is currently not known how the reversal frequency is regulated except that cell-cell contacts may induce C-signal exchange which is supposed to stimulate reversals during rippling and to inhibit reversals during aggregation. During fruiting body formation the reversal frequency decreases up to a point where cell movements become nearly unidirectional [20] and cells start to display collective motion with the formation of large clusters in which cells are aligned in parallel making side-to-side as well as head-to-tail contacts and move in the same direction [21]. Eventually cells start to aggregate. Aggregation centers often resemble at their initial phase a cell vortex. Here, we aim at understanding myxobacterial pattern formation processes, particularly the contributions by the two motility machineries as well as the cell reversal machinery to the spatial organization of the cells. We study the role of steric interactions, cell adhesion, and reversal frequency on the collective dynamics. The question for us is not “why” cells exhibit a given collective behavior but “how” they do it. In order to identify the role of the two motility machineries and cell reversal machinery, we follow a bottom-up strategy by looking at the collective dynamics of different mutants of increasing complexity. We analyze three M. xanthus strains: i) a mutant that moves unidirectionally without reversing by the Amotility system only – mutant that has been previously studied by us in [7] –, ii) a unidirectional mutant that is also equipped with the S-motility system, and iii) the wild-type that, in addition to the two motility systems, occasionally reverses its direction of movement. We char- 3 acterize the macroscopic patterns mainly through the cluster statistics, in particular in terms of cluster size and shape. We observe that the mutant moving by means of the A-engine only displays collective motion in the form of large moving clusters. The study of its cluster size distribution reveals that above a given density, clusters can be arbitrary large [7]. Here, we show in addition that there is a non trivial scaling of cluster perimeter with cluster size which indicates that the clustering process is neither (fully) random nor as in (equilibrium) liquidvapor drops [10]. We also find that at high densities the collective dynamics changes and cells organize into vortices. The study of the two-engine strain mutant reveals the same phenomenology for these bacteria: collective motion in the form of large moving clusters, a critical density above which cluster can be arbitrarily large, a non-trivial scaling of cluster perimeter with cluster size, and vortex formation at high densities. From the comparison of these two strains, we conclude that unidirectional cell motion induces the formation of large moving clusters at low and intermediate densities, while it results into vortex formation at very high densities, see first and second row of panels in Fig. 1. Interestingly, similar collective dynamics has been observed in self-propelled rod models [11], a fact that strongly suggests that the combined effect of self-propulsion and volume exclusion interactions is the pattern formation mechanism leading to the observed phenomena. The study of wild-type cells indicates that cell reversal weakens clustering. Wild-type cells exhibit exponential cluster size distributions at low and intermediate densities, while the scaling of the cluster perimeter with cluster size indicates that clusters are strongly elongated. At high densities, we find that reversing wild-type cells selforganize into a mesh-like structure, see bottom row in Fig. 1. Wild-type cells, as commented above, exhibit a large variety of self-organized patterns depending on the environmental condition. Our results suggest that by only switching on and off the reversal, cells can modify dramatically their collective behavior, with the suppression of cell reversal leading to collective motion in the form of moving clusters and vortex formation at high densities. This observation is consistent with the observed decrease in reversal frequency in the wild-type upon nutrient depletion, which is followed by the formation of large moving clusters and aggregation of cells. Our findings indicate that these two processes can result from simple steric interactions of the (non-reversing) rod-shaped cells, without the need of invoking any biochemical signal regulation. The paper is organized as follows. In Sec.I.a, we focus on the spatial self-organization of purely A-motile cells in the absence of cell reversals. The effects induced by the S-motility engine, which include increased cell adhesion, are studied in Sec.I.b, while those due to cell reversals in Sec.I.c. In Sec.II we discuss which collective effects are expected in self-propelled rod models, and interpret the cluster statistics results observed in the experiments in the light of a simple cluster formation theory. We summarize all the results in Sec. III, where we also discuss the implications of the reported findings. I. A. CLUSTER STATISTICS A-motile non-reversing cells We start out with the simple mutant A+ S− Frz− that only moves by means of the A-motility system and which is unable to reverse due to an insertion in the frz gene cluster (see Material and Methods for more details about how the strain was generated). This mutant is unable to assemble type IV pili due to deletion of the pilA gene, which encodes the type IV pili subunit, and therefore the S-motility system is non-functional in this mutant. This mutant exhibits relatively weak cell-cell adhesion due to the lack of type IV pili and the reduced accumulation of exopolysaccharides. This mutant is labeled A+ S− Frz− to indicate that A-motility engine is on, the S-motility engine is off and the Frz system, i.e., cell reversal is dramatically reduced. Control experiments showed that these mutants have a reversal period 100 min whereas the isogenic Frz+ strain reversed with a mean reversal period of ∼ 10 min. In [7], we showed that this mutant exhibits a transition to a collective motion phase at high enough densities by analyzing the dependency of cluster size distribution with the packing fraction. Here, we characterize in addition the cluster shape, and show that at densities higher than the one studied in [7], giant clusters turn into vortices. Experiments were performed by spotting a drop of cell suspension of the desired density on an agar surface to subsequently monitor the evolution of cell arrangements by taking snapshots of the bacterial colony every 30 min for a total of 8 hrs. Experiments with cells gliding in isolation indicate an average velocity of v = 3.10 ± 0.35 µm/min, an average width of about W = 0.7 µm and an average length of L = 6.3 µm. This results in a mean aspect ratio of κ = L/W = 8.9 ± 1.95 and a cell covering an average area a = 4.4 µm2 . We found that under these conditions cells organized over time into moving clusters. Time-lapse recordings showed that collisions of cells lead to effective alignment (Fig. 2a). When the interaction is such that cells end up parallel to each other and move in the same direction, they migrate together for a long time (typically > 15 min). Eventually, successive collisions allow a small initial cluster to grow in size, Fig. 2. In the individual clusters, cells are aligned in parallel to each other and arranged in a head-to-tail manner, as previously described [24]. In a cluster, cells move in the same direction. Cluster-cluster collision typically leads to cluster fusion, whereas splitting and break-up of clusters rarely occur. On the other hand, individual cells on the border of a cluster often spontaneously escape from the cluster. 4 FIG. 2: (a) Collisions among M. xanthus lead to an effective (local) alignment. (b) and (c) show that a local alignment leads to formation of moving clusters; arrows indicate the cluster moving direction. Time interval between (b) and (c) is 15 min, snapshots correspond to A+ S− Frz− cells at packing fraction η = 0.11. Panels taken from [7]. These two effects, cluster growth due to cluster-cluster collision and cluster shrinkage, mainly due to cells escaping from the cluster boundary, compete and give rise to a characteristic cluster size distribution (CSD). The CSD - p(m, t) - indicates the probability of a bacterium to be in a cluster of size m at time t. Note that along the text, the term CSD always refers to this definition. Often times the cluster size distribution is alternatively determined as the number nm (t) of clusters of size m at time t. There is a simple relation between these two definitions: pm (t) ∝ m nm (t). In experiments we have observed that the CSD mainly depends on the packing fraction η, where η = ρ a, with ρ the (two-dimensional) cell density and a the average covering area of a bacterium given above. Hence, for all snapshots first the packing fraction was determined. Then, images with similar packing fraction η were compared and the CSD was reconstructed by determining the CSD for all images within a finite interval of the packing fraction. Very importantly, we find that the CSD p(m, t) reaches a steady state p(m) after some transient time, as shown in Fig. 3. We conclude that the clustering process evolves towards a dynamic equilibrium, where the process of formation of cell clusters of a given size is balanced by events in which clusters of this size disappear by either fusing with other clusters or by loosing individual cells from their boundary. The steady-state CSD p(m) strongly depends on the packing fraction η, with more and more cells moving in larger clusters for increasing packing fraction η. This is evident in Fig. 4, where we observe that at small values of η, p(m) exhibits a monotonic sharp decay with m, while at large η values, p(m) is non-monotonic, with an additional peak at large cluster sizes. The solid curves in Fig. 4 are fitted to the raw data by using phenomenological functional forms described in the next section. The CSD here was determined at a fixed time (450 minutes) after the beginning of each experiment; control experiments at other times (360 minutes, 480 minutes) revealed practically identical behavior. We interpret the presence of a peak at large values of m at bigger values of the packing fractions as the emergence of collective motion resulting in formation of large clusters of bacteria mov- ing in a coordinated fashion. The clustering transition is evident by the functional change displayed by p(m), monotonically decreasing with m for small values of η, while exhibiting a local maximum at large η values. At a critical value ηc = 0.17 ± 0.02 that separates different regimes of behavior, the CSD can be approximated by p(m) ∝ m−γ0 , with γ0 = 0.88 ± 0.07. Control experiments with non-motile cells do not exhibit a power-law behavior in the CSD. For more details, we refer to reader to [7]. Hence, we conclude that without active motion of cells no comparable transition to clustering occurs. In other words, active motion is required for the dynamical self-assembly of cells. Now, we turn our attention to the cluster shape, in particular to the scaling of the cluster perimeter Π(m) with the cluster size m. This kind of information can help us to realize how adhesive cells are and which role adhesion plays in the clustering process. If there is surface tension, then cluster should tend to minimize their surface, and they should be round, as observed in liquidvapor drops [10]. On the other hand, if surface tension is negligible, cluster can be very elongated object, with most of the cells on the cluster boundary, and the cluster perimeter is proportional to cluster size. We assume that Π(m) ∝ mω , where m denotes the area of the cluster. Thus it is clear that perimeter exponent ω should be 0.5 for round clusters. This would be the case for very adhesive cells exhibiting random movements. If clusters are extremely elongated, then ω = 1. We notice that ω = 1 would correspond also a fully random process as observed in percolation theory [10]. In short, the exponent ω is then such that 0.5 ≤ ω ≤ 1. Fig. 5 shows that for A+ S− Frz− cells ω = 0.60 ± 0.03, which indicates that the clustering process is non trivial that it neither fully random nor dominated by surface tension, see also Fig. 1. The scaling of Π(m) with m plays a central role in the clustering theory we discuss below, where the relation between cluster size statistics and cluster perimeter statistics will be discussed in detail. As the density increases, typical above η > 0.26, cells do not organize into large moving clusters, and giant clusters evolve into vortices. These vortices are formed by one or several layers of rotating disks whose radii dimin- 5 FIG. 3: Time convergence towards a steady state. The figure compares the cumulative cluster size distribution (CCSD), defined as p(x <= m), at various time points for A+ S− Frz− and A+ S+ Frz− cells at two different packing fractions. The CCSD is less noisy than the CSD and the comparison at various time points becomes possible. The first row, corresponding to A+ S− Frz− cells, indicates that the cluster statistics quickly converges to a steady state. The time convergence for A+ S+ Frz− cells, second row, also occurs, though the phenomenon is less evident. Each panel shows, as reference, the CCSD obtained with control experiments of non-motile cells. The comparison indicates that cell motility promotes undoubtedly the formation of large clusters. FIG. 4: Asymptotic cluster size distribution (t = 450 min) at various packing fractions η for non-reversing mutants A+ S− Frz− and A+ S+ Frz− and A+ S+ Frz+ . The three strains exhibit a cluster dynamics that evolves towards a steady cluster size distribution which is function of the cell packing fraction. The cluster size distribution (CSD) for A+ S− Frz− and A+ S+ Frz− cells exhibits a qualitative change at a critical packing fraction ηc ∼ 0.17; for η > ηc the CSD is no longer monotonically decreasing distribution and a peak at large cluster sizes emerges. At the critical point, p(m) ∝ m−ξ , with ξ ∼ 0.88. The CSD of the densities examined can always be approximated by a power-law with an exponential cut-off. Reversing, fully motile A+ S+ Frz+ cells (wild-type) display an asymptotic CSD which is for all packing fractions η < η ∗ exponential. For η > η ∗ , clusters connect such that cells form a mesh-like structure as shown in Fig. 1. ish the higher the disk is located in the z-direction. Fig. 6 shows a typical example of vortex formation; see the supplementary material for a movie and [59] for a brief description of the movie. Notice that these vortices are not disordered aggregates of cells as suggested in [25]. Given the fact that vortices are multilayered structures, phase contrast imaging can only provide limited information regarding the actual cell arrangements inside vortices. A detailed study of vortices requires more sophisticated experimental techniques. 6 Interestingly, vortex formation has been also observed in other experimental “self-propelled rod” systems as actin-myosin motility assays [26, 35] as well as in 2D suspensions of sperms [27]. In the later example, hydrodynamical interactions are supposed to induce the observed pattern, while in the former ones the role of hydrodynamic interactions is not well understood; yet in both type of systems the vortex patterns correspond to vortex arrays. In myxobacteria, on the other hand, hydrodynamical effects can be neglected and vortices do not emerge in a lattice-like arrangement, but rather in a disorganized fashion. At a theoretical level, vortices has been found in active gel theory [57, 58]. Wether active gel vortices and those observed in M. xanthus mutants have the same microscopic origin is unclear, but certainly a possibility worth exploring. In summary, the finding of vortex formation in experiments with A+ S− Frz− indicates that the S-motility system, cell-to-cell signaling, and cell reversals are not required for the organization of cells into vortices. B. A- and S-motile, non-reversing cells We turn our attention to the next simplest mutant: A+ S+ Frz− . These cells contain both motility engines found in the wild-type, while cell-reversals are absent. The S-motility system depends on type IV pili [17]. It allows cells to move in a contact-dependent manner, i.e. cells have to be in close proximity for S-motility to become active. As previously reported [17], we find that A+ S+ Frz− cells are more adhesive. Our aim is to understand whether the S-motility engine affects the spatial self-organization of cells. We performed the same analysis on A+ S+ Frz− cells as described for A+ S− Frz− cells and investigate cell densities close to the obtained critical density. Fig. 1 shows that at least at first glance the cluster statistics resembles that obtained with A+ S− Frz− cells. This suggests that the additional motility including its adhesion effect has no significant impact on the organization of cells within a cluster. By looking in more detail on the clustering data some subtle differences can be revealed. We observe that for all fixed packing fractions η, the CSD seems to evolve towards a steady state, Fig. 3. However, the temporal convergence is slower than the one observed for A+ S− Frz− cells. Assuming that CSD after 450 min from the beginning of the experiment is representative of the steady state CSD, we show in Fig. 4 the asymptotic behavior of the CSD with packing fraction η. The CSDs of the packing fractions η < 0.18 can be roughly approximated by a power-law, p(m) ∝ m−γ0 , with a critical exponent γ0 consistent with the one obtained for A+ S− Frz− cells, i.e., 0.81 ≤ γ0 ≤ 0.95, see Fig. 4. On the other hand, the data indicates that a local maximum, as the one described above for A+ S− Frz− , emerge for η ≥ 0.18, Fig. 4. On the other hand, the cluster shape statistics shows that the scaling of the perimeter Π with the cluster mass m is again consistent with the one obtained for A+ S+ Frz− cells with ω = 0.62 ± 0.03, see Fig. 5. Finally, at sufficiently high densities, these cells also self-organize into vortices. C. Wild-type and the effect of cell-reversal We applied the same analysis to the reversing A+ S+ Frz+ cells that move by means of both motility systems. Fig. 1 shows that the spatial organization of wild-type cells is dramatically different from the one observed in the two mutants. Undoubtedly, cell-reversal has a strong impact on the macroscopic behavior of the colony. The CSD distribution after 450 min is exponential for all η < 0.20 as shown in Fig. 4. The net distance of cell movement is reduced due to cell reversals and cells can only form small clusters. On the other side, clusters exhibit a more elongated shape than those found in experiments with A+ S− Frz− and A+ S+ Frz− cells, as confirmed by the scaling of the perimeter Π(m) which is characterized by a very different exponent ω = 0.82 ± 0.03, see Fig. 5. The initial monodisperse phase, characterized by an exponential CSD and very elongated clusters, undergoes a transition at packing fractions larger than 0.26. The new arrangement of cells percolates and the cells organize into a mesh-like structure, as shown in Fig. 1. II. KINETIC MODEL FOR THE CLUSTER STATISTICS In the following, we outline a generalized kinetic model for the cluster-size distribution and compare it to the above experimental results. In particular, we want to relate the cluster size distribution data and the cluster shape statistics. The model equations are built on the well-established coagulation theory for colloidal particles originally suggested by Smoluchowski [31], for an early review see also [32]. A similar phase transition (albeit with different exponents for the cluster-size distribution at criticality) was recently obtained in in a model for reversible polymerization representing a different generalization of the Smoluchowski model [33]. The model studied consists of a system of kinetic equations for the dynamics of the number nj (t) of clusters of size j at time t. It was first proposed in [11] to describe clustering in simulations of self-propelled rods. The individual cluster dynamics [? ], as well as the cluster-cluster dynamics [11, 34] are strongly simplified in this kinetic theory where the time evolution of the number nj (t) of 7 FIG. 5: Cluster perimeter π(m) as function of the cluster size m for three bacterial strains. The A+ S− Frz− and A+ S+ Frz− mutants exhibit roughly the same scaling π(m) ∝ mω , with ω ∼ 0.62 for the A+ S− Frz− , ω ∼ 0.60 for the A+ S+ Frz− , suggesting that an increase in adhesion does not have a strong impact on the cluster shape. On the other hand, cell reversals lead to much more elongated clusters, as the scaling of the A+ S+ Frz+ cells indicates, with ω ∼ 0.82. We have assumed that aggregation of cells occurs only due to cluster-cluster collisions. Following earlier work [11, 34], the collision rate between clusters of mass j and k is defined by: √ v0 σ 0 p Aj,k = j+ k , (3) δ FIG. 6: Vortex formation (circular pattern in the center) in the non-reversing mutant A+ S− Frz− at high cell density (η > 0.26). The pattern consists of rotating stacked discs of cells. These structure are observed in both, A+ S− Frz− and A+ S+ Frz− strains. Bj = clusters of size j is simply given by: ṅ1 = 2B2 n2 + N X Bk nk − k=3 N −1 X Ak,1 nk n1 k=1 ṅj = Bj+1 nj+1 − Bj nj − N −j X Ak,j nk nj k=1 j−1 1X + Ak,j−k nk nj−k 2 for j = 2, ....., N − 1 k=1 ṅN = −BN nN + N −1 1 X Ak,N −k nk nN −k , 2 (1) k=1 where the dot denotes a time derivative and N is the total number of cells in the system. The cluster-size distribution is then simply obtained from p(m, t) = m nm (t) . N where v0 represents the average speed of individual cells, σ0 is the average scattering cross section a single√cell √ of √ which is assumed to be σ0 ≈ L + W = a( κ + 1/ κ) and δ is the total area of the system. Eq. (3) assumes that cluster have a well-defined direction of motion, which means that the equation is not adequate to describe cluster-cluster coagulation in experiments with wild-type cells. This process competes with cluster fragmentation stemming from the escape of individual single cells from the cluster boundary. The fragmentation rate is given by the expression (2) v0 j ω v0 j ω √ , = R0 L R0 aκ (4) where R0 is a proportionality constant that is the only free parameter in the theory that is used to fix the critical value ηc ∝ R0−1 at the same values as in the experiment. The exponent ω in the fragmentation rate has an important role: it represents the scaling between the cluster mass m and the cluster perimeter Π, i.e., Π ∝ mω . If one assumes large clusters of approximately circular shape, then ω = 1/2; this special case has been previously studied in [11]. If instead one considers that cells form elongated narrow clusters, where practically all cells are near the boundary, then a choice of ω = 1 is appropriate. In practice, the value of ω will depend on the number j of particles in the respective cluster. For simplicity, we study only the limiting cases ω = 1/2 and ω = 1 and compare the resulting cluster-size distribution to the experimental findings. According to the model, the exponent γ only depends on the scaling of Π(m), i.e., the exponent ω, while the critical packing fraction 8 ηc is a non-universal quantity. The analysis of Eqs. (1), performed by direct numerical integration using a fourthorder Runge-Kutta method, reveals that for η ≤ ηc , the scaling of p(m) takes the form: p(m) ∝ m−γ0 exp(−m/m0 ) , (5) while above it, i.e., for η > ηc , the scaling is: p(m) ∝ m−γ1 exp(−m/m1 ) + Cmγ2 exp(−m/m2 ) , (6) with γ1 , γ2 , m1 , m2 and C constants that depend on η and system size. Eq. (5) is the result of a system size study of Eqs. (1) at the critical point (not shown), while Eq. (6) is just an educated guess. Eqs. (5) and (6) have been used to fit the experimental data for the cluster size distributions in the different strains of myxobacteria shown in Fig. 4. For η < ηc , for either A+ S− Frz− and A+ S+ Frz− cells we find using Eq. (5) γ0 ∈ [0.80, 0.95] and m0 ∈ [20, 1300] (m0 ∼ 20 for η = 0.04 and m0 ∼ 1300 for η = 0.16). Nevertheless, the critical exponent γ0 has been estimated by the method explained in the Material and methods section, where γ0 is found to be γ0 = 0.88±0.07. For wild-type cells, the distribution is strongly dominated by an exponential tail. Using Eq. (5) we find γ0 ∈ [0, 0.63] and m0 ∈ [10, 120]. Through Eq. (1), it can be shown that m0 is a function of η that increases as ηc is approached from below as observed in Fig. 4. According to the kinetic model, the critical packing fraction ηc is defined by p(m) ∝ m−γ0 at η = ηc as long as m is below the total number of cells N in the system. In contrast, for η < ηc the function p(m) clearly exhibits an exponentially decaying tail at larger m, as observed in the experiments with A+ S− Frz− and A+ S+ Frz− cells, Fig. 7. The theoretical CSD p(m, t) was obtained by numerical integration from an initial condition with n1 = N and ni = 0 for i ≥ 2. The values of the variables ni of Eq. (1) reached constant steady values after sufficiently large integration times. The steady state p(m) was found to depend only on the packing fraction η for a given perimeter scaling characterized by ω. For both values of ω studied, we find a transition from an exponentially decaying CSD, described by Eq. (5) for low densities, to a non-monotonic CSD, described by Eq. (6), consisting of a power-law behavior for small cluster sizes and a peak, local maximum, at large cluster sizes, see Fig. 7. Upon closer inspection of the model results, one recovers distinctly different exponents for the different model assumptions regarding ω: γ0 = 1.3 for ω = 1/2 and γ0 = 0.85 for ω = 1. Both choices of ω give reasonable qualitative agreement with the experimental data shown in Fig. 4 above, see Fig 7. Moreover, we find that the exponent of the cluster-size distribution is nonuniversal and depends sensitively on the choice of the fragmentation rate in Eq. (4). We expect that changes in the collision rate for the cluster will have a similarly strong effect, as discussed below. The clustering model given by Eq. (1) allows to study the relationship between the perimeter scaling (charac- terized by an exponent ω) and the cluster size distribution exponent γ0 . Eq. (1) also predicts the existence of two CSDs, depending on the the packing fraction η, i.e., Eqs. (5) and (6). These two predicted distributions are found in experiments with A+ S− Frz− and A+ S+ Frz− cells. For the wild type cells, only the CSD given by Eq. (5) is found. In this context, it is interesting to note that the results shown in Fig. 7 imply that for ω = 1 one needs to assume a much lower fragmentation rate - indicated by a much larger value of the parameter R0 than for ω = 0.5 to obtain the same critical ηc . Beyond the apparent agreement between the CSD exhibited by Eq. (1) and the experimentally obtained CSDs for A+ S− Frz− and A+ S+ Frz− cells, there are important differences. To obtain a critical exponent γ0 close to 0.88, ω has to be large, specifically, close to 1, while the experimental measurements on Π(m) revealed ω ∼ 0.6. There are several possibilities that could explain this discrepancy. For instance, the assumption that the cluster-cluster coagulation is proportional to square root of the cluster mass has to be revised. An estimation of the scaling of the effective scattering cross section of a cluster with its mass, as well as an accurate measurement of the functional dependency of cluster speed with cluster mass would allow us to determine the correctness of Eq. (1). Unfortunately, such measurements are extremely difficult to obtained. Nevertheless, the apparent discrepancy suggests that a possible generalization of the presented clustering theory would include a modification of Eq. (3). III. DISCUSSION In order to identify the role of the two motility machineries as well as cell reversal machinery on the spacial collective dynamics of M. xanthus, we have analyzed three bacterial strains: i) a mutant that moves unidirectionally without reversing by the A-motility system only, ii) a unidirectional mutant that is also equipped with the S-motility system, and iii) the wild-type that is equipped with the two motility systems and occasionally reverses its direction of movement. The study of the two non-reversing mutants revealed the same phenomenology. At low and intermediate densities, nonreversing cells displays collective motion in the form of large moving clusters, with a critical density above which clusters can be arbitrarily large. At the critical density, the two non-reversing strains exhibit a cluster size distribution characterized by roughly the same critical exponent γ0 ∼ 0.88. Even though the two-engine strain is supposed to be more adhesive than the single A-engine strain, we found a similar non-trivial scaling of cluster perimeter with cluster size characterized by an exponent ω ∼ 0.6. This finding indirectly shows that the clustering process is, for both stains, neither fully random nor an equilibrium one as in liquid-vapor drops [10]. In order to connect the statistics on cluster size and cluster shape, we derived a Smoluchowski-coagulation theory 9 FIG. 7: Theoretical predictions for the cluster size distribution (CSD). The cluster size distribution from the kinetic model depends on the scaling of the fragmentation Bm ∝ m−ω (see text). The figure shows the results for the two limiting cases, in the left panel ω = 0.5 (and R0 = 0.58) corresponding to round clusters, while in right panel ω = 1 (and R0 = 11.9), implying elongated clusters. Notice that in theory, as well as in experiments, the CSD can be well approximated by a power-law at the critical packing fraction ηc , while for η > ηc a peak at large cluster sizes emerges, a signature of dynamic self-assembly into larger moving clusters. Other model parameters: κ = 9, a = 4.4µm2 , and δ = 699 × 522µm2 with fragmentation, where we related the scaling of cluster perimeter with cluster size with the fragmentation kernel. The proposed theory allows us to understand the cluster formation process in absence of adhesion as a dynamic self-assembly process. It predicts the existence of a steady state cluster size distribution which is function of the cell density and perimeter exponent ω, and a functional change of the cluster size distribution above a critical density. In addition, the proposed theory predicts that the critical exponent γ0 depends on the perimeter exponent ω only. In summary, the theoretical clustering model provides a qualitative descriptions consistent with the experimental measurements, and explains why if the value of ω is similar for both strains, the value of γ0 has to be also similar. We observe that similar spatial organization has been observed in self-propelled rod simulations using either rigid [11] or elastic [28] elongated particles. We found that at high densities the collective dynamics changes and cells organize into vortices. This finding cannot be account by the proposed clustering theory, but it is reminiscent of what is observed in self-propelled rod simulations at high densities, though in experiments vortices seem to be stable structures while in simulations vortices are unstable. From the comparison of these two non-reversing strains, we conclude that unidirectional cell motion induces the formation of large moving clusters at low and intermediate densities, while it results into vortex formation at very high densities. On the light of the clustering theory and given the remarkable similarity with self-propelled rod simulations, we suggest that the spatial self-organization in these two strains occurs in absence of biochemical signal regulations and as result of the the combined effect of self-propulsion and volume exclusion interactions. All these results strongly suggest that the combination of self-propulsion and steric interaction is a valid pattern formation mechanism which could be also at play in recent experiments with Escherichia coli [45] and driven actin filaments [35], which makes us wonder about the connection between this mechanism and the large body of work on simple models of selfpropelled particles where spontaneous segregation and long-range orientational has been reported [36–44]. The study of wild-type cells has revealed that cell reversal affects dramatically the collective dynamics. We found that wild-type cells exhibit cluster size distributions exponentially distributed at low and intermediate densities. On the other hand, we measured an the scaling of the cluster perimeter with cluster size characterized by a large exponent ω ∼ 0.8 which indicates that clusters are strongly elongated with comparison to those found in experiments with the two non-reversing mutants. Finally, we observed that at high densities cells self-organize into a mesh-like structure. A qualitative understanding of this macroscopic behavior is still missing. The comparison of the two non-reversing strains and wild-type cells suggest suggests that by only switching on and off the reversal, cells can modify dramatically their collective behavior, with the suppression of reversal leading to collective motion in the form of moving clusters and vortex formation at high densities. We note that this observation is consistent with the observed decrease in reversal frequency in the wild-type upon nutrient depletion, which is followed by the formation of large moving clusters and aggregation of cells. At a more speculative level, our results suggest that the cell density and the rod shape of the cells may play an essential role for bacteria to achieve collective motion [46, 47]. According to self-propelled rod simulations, an elongated cell shape strongly facilitates collective motion by promoting the formation of larger clusters. Another hint that the rod-shape of the moving bacteria is important for collective motion is provided by the empirical observation that many bacteria undergo a dramatic elongation of their cell shape before assembling 10 into larger groups, e.g. in Vibrio parahaemolyticus [48] or B. subtilis [49]. Finally, the reported results increase the plausibility of earlier biological hypotheses [46], that multicellular organization may be achieved by regulating the cell density via proliferation and cell length by direct developmental control. We acknowledge support by the German Ministry for Education and Research (BMBF) through grants no. 0315259 and no. 0315734, by the Human Frontier Science Program (HFSP) through grant no. RGP0016-2010, by DFG through grant DE842/2 and the Max Planck Society. Partial DFG support by SFB 555 and GRK 1558 is also acknowledged. AD is a member of the DFG Research Center for Regenerative Therapies Dresden – Cluster of Excellence – and gratefully acknowledges support by the Center. FP acknowledges support by PEPS PTI “Anomalous fluctuations in the collective motion of self-propelled particles”. IV. MATERIAL AND METHODS A. Bacterial strains. The fully motile strain DK1622 (A+ S+ Frz+ ) was used as a wild type [50] and all other strains used are derivatives of DK1622. The non-reversing strain DK8505 [51] is referred to as A+ S+ Frz− . To generate SA2407 cells, here referred to as A+ S− Frz− , the frz loss-of-function allele f rzCD::T n5 lac Ω536 from DK8505 [51] was introduced into the ∆pilA strain DK10410 [52], which is unable to assemble type IV pili, using standard procedures [53]. To generate SA2082 (∆pilA, romR::nptII), the nonmotile M. xanthus mutant referred to as A− S− Frz− , the romR::nptII loss-of-function allele from SA1128 [54] was introduced into DK10410. All strains used had a doubling time of approximately 5 hrs in CTT liquid medium at 32◦ C. Notice that the relaxation time of spatial patterns is below 120 min which implies that the doubling time has a weak effect on the spatial patterns. B. Cluster formation experiments Cultures of M. xanthus were grown in CTT liquid medium [55] at 32o C with shaking to an estimated density of 7 × 109 cells/ml. Subsequently, cells were diluted to densities of 0.5 × 108 /ml, 1.0 × 108 /ml, 1.5 × 108 /ml, 1.75 × 108 /ml and 2 × 108 /ml, respectively. Cell densities were confirmed by colony counts on CTT agar plates manually and by counting the number of cells using a counting chamber manually. 30µl aliquots of cells were transferred to a microscope slide covered with a 1.0% agar pad in 0.5% CTT medium. The time point at which the cell drop was completely absorbed in the agar was set as t = 0. For each cell density, 16 slides were prepared and every 30min (starting at 30min) up to 480min, a sample was analysed by microscopy using a Leica DM6000B microscope with a Leica 20× phase-contrast objective and imaged with a Leica DFC 350FX camera. 20 phasecontrast images were taken at 20× magnification across a spot. After 480min a short time-lapse movie was taken to verify that cells and clusters were migrating. C. Image analysis Clustering images were taken at 20× magnification. Images contain cell clusters as dark regions, often surrounded by a light halo. Cluster boundaries were detected in a multi-step processing queue. After initial image normalization, edge detection via the Canny-Deriche algorithm was applied for two different levels of spatial detail. Both edge images were superimposed subsequently. Next, edges were filtered out that surround halos and other non-cluster objects. Finally, all incomplete detections were revised/corrected manually in a post-processing step. The areas of the clusters in pixels were extracted using an implementation of the processing queue in the image processing tool ImageJ (http://rsbweb.nih.gov/ij/). The number of cells inside a cluster, i.e., the cluster size, was estimated as the area of a cluster divided by the mean area covered by a single cell, which was found to be 150 pixels at 20-fold magnification. According to this definition, a cluster is a connected group of cells, regardless of their orientation. Packing fraction estimates per image were obtained as the ratio of area covered by cells and the whole area of the image (1392 × 1040 pixels corresponding to 699µm × 522µm). D. Statistical analysis After applying the image analysis procedure described above to a given image I, corresponding to a given packing fraction, a large array of various cluster sizes is obtained, and nI (m, t) can be computed. We represent by nI (m, t) the number of clusters of size m in the image I. To build the CSD we make use of all the available images corresponding to the given packing fraction η. Let the auxiliary function gI (m, t) be gI (m, t) = m nI (m, t). The average of this function reads: g(m, t) = (1/M ) X gI (m, t) , (7) I where M is the number of available images. To cope with the sparseness of the data for large cluster sizes we implemented several binning procedures, in particular, linear and exponential binning. In the following we explain the exponential binning procedure. The cluster size space is divided into bins, the first bin contains all clusters of size s, 0 < s ≤ 1, the second bin all clusters of size 1 < s ≤ 2, the third bin, 2 < s ≤ 4,... the n-th bin contains cluster 11 FIG. 8: Procedure to estimate the critical exponent γ0 and critical packing fraction ηc . a) The standard deviation of the transformation given by Eq. (10) with respect to its mean value W , see Eq. (11). The shown data corresponds to A+ S− Frz− cells. The minimum exhibited by η = 0.16 − 0.18 indicates that the transformation given by Eq. (10) leads to a horizontal line, indirectly showing that the values of η can be well fitted by Eq. (5). b) shows the sensitivity of this procedure. If the critical exponent is either overestimated or underestimated, there is no transformed CSD, for any value of η, yielding a horizontal line. Only very close to the actual critical exponent γ0 , the transformation can be approximated by a constant W . sizes 2n−1 < s ≤ 2n . It is useful to define the function: following transformation yields to a constant: e(n+1) gbin (n, t) = X X e(n) gI (m, t) (8) y(m) = p(m; ηc )mγ = W (9) where W is a constant and the equality holds true for 1 < x < xcut−of f , where xcut−of f denotes the beginning of the cut-off. The value of W is the average value of y(m) in the interval 1 < x < xcut−of f . This means that if we plot y(m) vs. m, we observe a horizontal line at the critical packing fraction ηc . We can measure how close we are to the horizontal line by computing: I where e(n) = 2n . The binned CSD is defined as: pbin (e(n), t) = (10) gbin (n, t) . C(e(n − 1) − e(n)) P Thus, m pbin (m = e(n), t)(e(n − 1) − e(n)) = 1. It is worth noticing that if the underlying CSD p(m) is a power-law characterized by an exponent γ, i.e., p(m) ∼ m−γ , the exponential binning procedure given by Eq. (9) results in pbin (m) ∼ m−γ . On the other hand, if the underlying CSD p(m) is an exponential, i.e., p(m) ∼ exp(m/m0 ), the exponential binning leads to pbin (m) ∼ m−1 exp(m/m0 ). In the text, for simplicity we referred to pbin (m, t) just as p(m, t). In what follows, we explain how the critical exponent has been measured. At the critical packing fraction ηc the CSD is a power-law (with an exponential cut-off due to the finite number of cells). The problem consists in identifying the critical packing fraction ηc and the critical exponent γ0 . Assuming that we know γ0 at ηc the [1] Bretschneider T, Siegert F, Weijer CK (1995) Threedimensional scroll waves of cAMP could direct cell movement and gene expression in Dictyostelium slugs. Proc. Natl. Acad. Sci. USA 92:4387-4391. [2] Ben-Jacob E, Cohen I, Levine H (2000) Cooperative self- σ 2 (η, γ) = X (y(m) − W )2 (11) By minimizing Eq. (11) with respect to η and γ, the critical packing fraction and critical exponent can be obtained. Figure 8 illustrates the procedure. In the figure the cut-off was taken to xcut−of f = 220 (various other values were also studied). We found that the critical packing fraction lays between 0.16 and 0.18 for either A+ S− Frz− or A+ S+ Frz− cells and the critical exponent is γ0 = 0.88 ± 0.07 and γ0 = 0.85 ± 0.07 for A+ S− Frz− or A+ S+ Frz− cells, respectively. organization of microorganisms. Adv. Phys. 49:395-554. [3] Kaiser D (2003) Coupling cell movement to multicellular development in myxobacteria. Nat. Rev. Microbiol. 1:4554. [4] Dombrowski C, Cisneros L, Chatkaew S, Goldstein 12 [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] [16] [17] [18] [19] [20] [21] [22] [23] [24] RE, Kessler JO (2004) Self-concentration and largescale coherence in bacterial dynamics. Phys. Rev. Lett. 93:098103. Zhang HP, Be’er A, Florin E-L, Swinney HL (2010) Collective motion and density fluctuations in bacterial colonies. Proc. Natl. Acad. Sci. USA 107:13626-13630. M. E. Cates et al. (2012). Arrested phase separation in reproducing bacteria: a generic route to pattern formation?. Proc. Natl. Acad. Sci. U.S.A. 107, 11715-11720. F. Peruani, J. Starruß, V. Jakovljevič, L. SøgaardAndersen, A. Deutsch, and M. Bär (2012) Collective motion and nonequilibrium cluster formation in colonies of gliding bacteria, Phys. Rev. Lett., 108, 098102. Whitesides GM, Grzybowski B (2002) Self-assembly at all scales. Science 295:2418–2421. Copeland MF, Weibel DB (2009) Bacterial swarming: a model for studying dynamic self-assembly. Soft Matter 5:1174-1187. D. Stauffer (1979), Scaling theory of percolation clusters, Phys. Rep 54, 1-74 . Peruani F, Deutsch A, Bär M (2006) Nonequilibrium clustering of self-propelled rods. Phys. Rev. E 74:030904030908(R). Yang Y, Marceau V, Gompper G (2010) Swarm behavior of self-propelled rods and swimming flagella. Phys. Rev. E 82:031904. Kudrolli A, Lumay G, Volfson D, Tsimring LS (2008) Swarming and swirling in self-propelled granular rods. Phys. Rev. Lett. 100:058001. Stevens A, Søgaard-Andersen L (2005) Making waves: Pattern formation by a cell surface-associated signal. Trends Microbiol. 13:249-252. Vos M, Velicer GJ (2006) Genetic population structure of the soil bacterium Myxococcus xanthus at the centimeter scale. Appl. Environ. Microbiol. 72:3615-3625. Mauriello EM, Mignot T, Yang Z, Zusman DR (2010) Gliding motility revisited: how do the myxobacteria move without flagella?. Microbiol. Mol. Biol. Rev. 74:229249. Wu SS, Kaiser D (1995) Genetic and functional evidence that Type IV pili are required for social gliding motility in Myxococcus xanthus. Mol. Microbiol. 18:547-558. Hodgkin J, Kaiser D (1979) Genetics of gliding motility in Myxococcus xanthus: two gene systemss control movement. Mol. Gen. Genet. 171:177-191. Blackhart BD, Zusman DR (1985) Frizzy genes of Myxococcus xanthus are involved in control of frequency of reveral of gliding motility. Proc. Natl. Acad. Sci. USA 82:8771-8774. Jelsbak L, Søgaard-Andersen L. (2002) Pattern formation by a cell surface associated morphogen in M. xanthus. Proc. Natl. Acad. Sci. USA 99:2032-2037. O’Connor KA, Zusman DR (1989) Patterns of cellular interactions during fruiting-body formation in Myxococcus xanthus. J. Bacteriol. 171:6013-6024. Wolgemuth C, Hoiczyk E, Kaiser D, Oster G (2002) How myxobacteria glide. Curr. Biol. 12:369–377. Mignot T, Shaevitz JW, Hartzell PL, Zusman DR (2007) Evidence of focal adhesion complexes power bacterial gliding motility. Science 315:853-856. Pelling AE, Li Y, Cross SE, Castaneda S, Shi W, Gimzewski KJ (2006) Self-organized and highly ordered domain structures within swarms of Myxococcus xanthus, Cell Motil. Cytoskeleton 63: 141–148. [25] Holmes AB, Kalvala S, Whitworth DE (2010) Spatial simulations of myxobacterial development. PLoS Comput Biol 6(2): e1000686. [26] Sumino Y. et al. (2012) Large-scale vortex lattice emerging from collectively moving microtubules. Nature 483, 448-52 [27] Riedel I., Kruse K., Howard J. (2007) A Self-Organized Vortex Array of Hydrodynamically Entrained Sperm Cells. Science 309, 300-303 [28] StarrußJ, Bley T, Søgaard-Anderson L, Deutsch A (2007) A new mechanism for collective migration in Myxococcus xanthus. J. Stat. Phys. 128:269–286. [29] Stevens A (2000) A stochastic cellular automaton, modeling gliding and aggregation of myxobacteria. SIAM J. Appl. Math. 61:172-182. [30] Sliusarenko O, Zusman DR, Oster G (2007) Aggregation during fruiting body formation in Myxococcus xanthus is driven by reducing cell movement. J. Bacteriol. 189:611– 619. [31] von Smoluchoswki M (1917) Versuch einer mathematischen Theorie der Koagulationskinetik kolloider Lösungen. Z. Phys. Chem. 92:129. [32] Chandrasekhar S (1943) Stochastic problems in physics and astronomy. Rev. Mov. Phys. 15:1–89. [33] Ben-Naim E, Krapivsky PL (2008) Phase transition with nonthermodynamic states in reversible polymerization. Phys. Rev. E 77:061132. [34] Peruani F., Schimansky-Geier L., and Bär M. (2010) Cluster dynamics and cluster size distribution in systems of self-propelled particles, Eur. Phys. J. Special Topics 191, 173-185. [35] Schaller V, Weber C, Semmrich C, Frey E, Bausch AR (2010) Polar patterns of driven filaments. Nature 467:73– 77. [36] Vicsek T, Czirok A, Ben-Jacob E, Cohen I, Shochet O (1995) Novel type of phase transition in a system of selfdriven particles. Phys. Rev. Lett. 75:1226. [37] Toner J, Yu Y (1995) Long-range ordder in a twodimensional XY model: How birds fly together. Phys. Rev. Lett. 75:4326. [38] Bussemaker HJ, Deutsch A, Geigant E (1997) Mean-field analysis of a dynamical phase transition in a cellular automaton model for collective motion. Phys. Rev. Lett. 78:5018. [39] Grégoire G., Chaté H. (2004) Onset of collective and cohesive motion. Phys. Rev. Lett. 92:025701. [40] Mishra S, Ramaswamy S (2006) Active nematics are intrinsically phase separated. Phys. Rev. Lett. 97:090602. [41] Ramaswamy S, Aditi Simha R, Toner J (2003) Active nematics on a substrate: giant number fluctuations and long-time tails. Europhys. Lett. 62:196. [42] Chaté H, Ginelli F, Grégoire G, Raynaud F (2008) Collective motion of self-propelled particles interacting without cohesion. Phys. Rev. E 77:046113. [43] Baskaran A, Marchetti MC (2008) Hydrodynamics of self-propelled hard rods. Phys. Rev. E 77:011920. [44] Ginelli F, Peruani F, Bär M, Chaté H (2010) Large-scale collective properties of self-propelled rods. Phys. Rev. Lett. 104:184502. [45] Drescher K, Dunkel J, Cisneros LH, Ganguly S, Goldstein RE (2011) Fluid dynamics and noise in bacterial cell-cell and cell-surface scattering. Proc. Natl. Acad. Sci. USA 108:10940–10945 [46] Young KD (2006) The selective value of bacterial shape. 13 Microbiol. Mol. Biol. Rev. 70:660–703. [47] Harshey RM (1994) Bees aren’t the only ones: swarming in Gram-negative bacteria. Mol. Microbiol. 13:389-394. [48] McCarter L (1999) The multiple identities of Vibrio parahaemolyticus. J. Mol. Microbiol. Biotechnol. 1:51–58. [49] Julkowska D, Obuchowski M, Holland IB, Seror SJ (2004) Branched swarming patterns on a synthetic medium formed by wild-type Bacillus subtilis strain 3610: detection of different cellular morphologies and constellations of cells as the complex architecture develops. Microbiology 150:1839-1849. [50] Kaiser D (1979) Social gliding is correlated with the presence of pili in Myxococcus xanthus. Proc. Natl. Acad. Sci. USA 76:5952. [51] Sager B, Kaiser D (1994) Intercellular C-signaling and the traveling waves of Myxococcus. Genes Dev. 8:2793. [52] Wu SS, Kaiser D (1997) Regulation of expression of the pilA gene in Myxococcus xanthus. J. Bacteriol. 179(24):7748. [53] Higgs PI et al. (2005) Four unusual two-component signal transduction homologs, RedC to RedF, are necessary for timely development in Myxococcus xanthus. J. Bacteriol. 187:8191. [54] Leonardy S, Freymark G, Hebener S, Ellehauge E, Søgaard-Andersen Lotte (2007) Coupling of protein localization and cell movements by a dynamically localized response regulator in Myxococcus xanthus. EMBO J. 26:4433. [55] Hodgkin J, Kaiser D (1977) Cell-to-cell stimulation of movement in non-motile mutants of Myxococcus. Proc. Natl. Acad. Sci. USA 74:2938. [56] Hodgkin J, Kaiser D (1979) Genetics of gliding motility in Myxococcus xanthus (Myxobacterales): Two gene systems control movement. Mol. Gen. Genet. 171:547–558. [57] J. Elgeti, M. E. Cates and D. Marenduzzo (2011) Soft Matter 7, 3177. [58] Kruse K., Joanny J. F., Julicher F., Prost J., and Sekimoto K., Asters (2004),Vortices, and Rotating Spirals in Active Gels of Polar Filaments, Phys. Rev. Lett. 92, 078101. [59] The movie shows a vortex of A+S-Frz- cells, magnification 20×, real time duration 15 min.